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相关论文: Dark Energy: Recent Developments

200 篇论文

Cosmological observations strongly suggest the presence of dark energy which comprises the majority of the current energy density of the universe. The equation of state relating the pressure and energy density of this dark energy, p = w…

天体物理学 · 物理学 2007-05-23 Eric Gawiser

A recently proposed Dynamical Space-time Cosmology (DSC) that unifies dark energy and dark matter is studied. The general action of this scenario includes a Lagrange multiplier, which is coupled to the energy momentum tensor and a scalar…

广义相对论与量子宇宙学 · 物理学 2019-06-10 Fotios K. Anagnostopoulos , David Benisty , Spyros Basilakos , Eduardo I. Guendelman

In the standard model of cosmology, the present evolution of the Universe is determined by the presence of two components of unknown nature. One of them is referenced as ``dark matter'' to justify the fact that it behaves cosmologically…

天体物理学 · 物理学 2007-05-23 Alexandre Arbey

The current paper provides a comprehensive examination of a dark energy cosmological model in the classical regime, in which a generic scalar field is regarded as a dark energy source. Einstein's field equations are solved in model…

广义相对论与量子宇宙学 · 物理学 2022-09-07 Ritika Nagpal , Shibesh Kumar Jas Pacif , Abhishek Parida

We discuss models that can account for today's dark energy. The underlying cosmological constant may be Planck scale but starts as a redundant coupling which can be eliminated by a field redefinition. The observed vacuum energy arises when…

高能物理 - 理论 · 物理学 2008-11-26 Puneet Batra , Kurt Hinterbichler , Lam Hui , Daniel Kabat

The cosmological constant, which was introduced by Einstein a century ago to allow for a static universe, experienced a revival two decades ago under the label dark energy as a parameter to model the observed accelerated expansion of the…

综合物理 · 物理学 2019-01-08 Jan O. Stenflo

Recent measurements suggest our universe has a substantial dark energy component, which is usually interpreted in terms of a cosmological constant. Here we examine how much the form of this dark energy can be modified while still retaining…

高能物理 - 唯象学 · 物理学 2009-11-07 Duane A. Dicus , Wayne W. Repko

We consider a model where both dark energy and dark matter originate from the coupling of a scalar field with a non-conventional kinetic term to, both, a metric measure and a non-metric measure. An interacting dark energy/dark matter…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Stefano Ansoldi , Eduardo I. Guendelman

Observational evidence for the existence of dark energy is strong. Here we suggest a model which is based on a modified gravitational theory in 5D and interpret the 5th dimension as a manifestation of dark energy in the 4D observable…

高能物理 - 理论 · 物理学 2008-01-22 H. Alavirad , N. Riazi

Here, creation of the universe is obtained only from gravity sector. The dynamical universe begins with two basic ingredients (i) vacuum energy, also called dark energy (as vacuum energy is not observed) and (ii) background radiation. These…

高能物理 - 理论 · 物理学 2007-05-23 S. K. Srivastava

Rapid progress has been made recently toward the measurement of cosmological parameters. Still, there are areas remaining where future progress will be relatively slow and difficult, and where further attention is needed. In this review,…

天体物理学 · 物理学 2009-10-31 Wendy L. Freedman

Quantum field theory predicts that vacuum energy (or what is the same, cosmological constant) should be 50-100 orders of magnitude larger than the existing astronomical limit. A very brief review of possible solutions of this problem is…

天体物理学 · 物理学 2007-05-23 A. D. Dolgov

This paper deals with a cosmological model in which the universe is filled with tachyon dark energy in order to describe current and future accelerating expansion. We obtain that the simplest condition for the regime of phantom energy to…

天体物理学 · 物理学 2009-11-10 Pedro F. Gonzalez-Diaz

The dominance of dark energy in the universe has necessitated the introduction of a repulsive gravity source to make q0 negative. The models for dark energy range from a simple lambda-term to quintessence, Chaplygin gas, etc. We look at the…

综合物理 · 物理学 2011-09-12 C. Sivaram , Kenath Arun , R. Nagaraja

Astrophysical observations are pointing out huge amounts of dark matter and dark energy needed to explain the observed large scale structures and cosmic accelerating expansion. Up to now, no experimental evidence has been found, at…

天体物理学 · 物理学 2009-11-11 S. Capozziello , V. F. Cardone , A. Troisi

A set of temporal singularities (transients) in the mass-energy density and pressure, bearing a specific mathematical structure which represents a new solution to the continuity equation (\ie~conservation of mass-energy) and satisfying the…

广义相对论与量子宇宙学 · 物理学 2025-03-13 Richard Lieu

An impressive amount of different astrophysical data converges towards the picture of a spatially flat universe undergoing a today phase of accelerated expansion. The nature of the dark energy dominating the energy content of the universe…

天体物理学 · 物理学 2009-11-10 S. Capozziello , V. F. Cardone , M. Funaro , S. Andreon

In this work, we study tracker phantom dark energy models with a general parameterization of the scalar potentials. Our analysis also considers the scenario of having both phantom field and the cosmological constant as the dark energy…

宇宙学与河外天体物理 · 物理学 2021-05-18 Francisco X. Linares Cedeño , Nandan Roy , L. Arturo Ureña-López

Observational evidence of dark energy that makes the Universe nearly flat at the present epoch is very strong. We study the link between spatial continuity and dark energy. We assume that comoving space is a compact 3-manifold of constant…

宇宙学与河外天体物理 · 物理学 2009-12-02 Boudewijn F. Roukema , Vincent Blanloeil

In the cosmological context an effective quantum field theory describing the behavior of visible matter in the universe is characterized with its inherent UV cutoff and also with an IR scale that is set by the cosmological (particle)…

高能物理 - 唯象学 · 物理学 2008-11-26 Michael Maziashvili